Abstract
Data derived from coronal eclipse spectra in the visible range are analyzed in terms of electron density and temperature in a coronal condensation using the method recently developed by Jefferies, Orrall and Zirker. A mean density and a certain amount of material are associated to each temperature. Abundances relative to Fe are derived for Ni, Cr, Mn, S, Ca. The absolute abundance of Fe is found to be 2 × 10−5. No absolute calibration is required. It appears that there must exist a non-negligible amount of ‘cold’ material (T e < 106K) in the corona, which cannot be observed in the visible spectral range.
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Magnant-Crifo, F. Absolute abundances and distribution of material versus density and temperature in a coronal condensation. Sol Phys 39, 141–151 (1974). https://doi.org/10.1007/BF00154976
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DOI: https://doi.org/10.1007/BF00154976